EVAT 554 OCEAN-ATMOSPHERE DYNAMICS EQUATIONS OF MOTION (CONT); ENERGY EQUATION LECTURE 4 (Reference: Peixoto & Oort, Chapter 3)

Slides:



Advertisements
Similar presentations
Introduction Irina Surface layer and surface fluxes Anton
Advertisements

Institut für Meteorologie und Klimatologie Universität Hannover
F.Nimmo EART164 Spring 11 EART164: PLANETARY ATMOSPHERES Francis Nimmo.
Section 2: The Planetary Boundary Layer
PTT 201/4 THERMODYNAMICS SEM 1 (2012/2013) 1. light Energy can exist in numerous forms: Thermal Mechanical Kinetic Potential Electric Magnetic Chemical.
AOSS 321, Winter 2009 Earth System Dynamics Lecture 10 2/10/2008 Christiane Jablonowski Eric Hetland
Vertical structure of the atmosphere. Review of last lecture Earth’s energy balance at the top of the atmosphere and at the surface. What percentage of.
Photosynthetically-active radiation (spectral portion, CI) h h h h h h h h.
Energy & Work. Energy What is energy? The capacity to do work What is Work? The transfer of energy from one physical system to another Bottom line: it.
5.7 PW5.9 PW The seasonal cycle of energy fluxes in the high latitudes Aaron Donohoe I.) How do the absorbed solar (ASR), outgoing longwave (OLR), and.
2-1 Problem Solving 1. Physics  2. Approach methods
CHE/ME 109 Heat Transfer in Electronics
ENAC-SSIE Laboratoire de Pollution de l'Air The Atmospheric Layers.
CE 318: Transport Process 2 (Heat and Mass Transfer) Lecture 18: Convective Mass Transfer (Chapter 28) NSC 210 4/16/2015.
Chapter 2 Energy in the Atmosphere. Energy It’s what makes things happen.
Energy Transfer By Heat, Work, and Mass
The General Circulation of the Atmosphere Background and Theory.
Atmospheric Analysis Lecture 2.
Conservation of Mechanical Energy Chapter 6. Energy  As you know, energy comes in many forms. Kinetic Energy Potential Energy  Gravitational Potential.
Dynamics Energetics of General Circulation In the previous lecture we discussed the characteristics of the general circulation of the atmosphere In today’s.
EVAT 554 OCEAN-ATMOSPHERE DYNAMICS THERMOHALINE CIRCULATION (CONTINUED) LECTURE 20.
Introduction to Numerical Weather Prediction 4 September 2012.
F.Nimmo EART164 Spring 11 EART164: PLANETARY ATMOSPHERES Francis Nimmo.
Evaporation Slides prepared by Daene C. McKinney and Venkatesh Merwade
General Circulation of the Atmosphere Lisa Goddard 19 September 2006.
Basic dynamics  The equations of motion and continuity Scaling Hydrostatic relation Boussinesq approximation  Geostrophic balance in ocean’s interior.
Aerodynamics Linear Motion (Moving Air ).
Surface energy balance (2). Review of last lecture –What is energy? 3 methods of energy transfer –The names of the 6 wavelength categories in the electromagnetic.
Evaporation What is evaporation? How is evaporation measured? How is evaporation estimated? Reading: Applied Hydrology Sections 3.5 and 3.6 With assistance.
METR February Review State variables: p, ρ, T Pressure Temperature Equation of state: p = NkT/V = ρ R d T Virtual temperature T v = T (1.
Reynolds-Averaged Navier-Stokes Equations -- RANS
Momentum Equations in a Fluid (PD) Pressure difference (Co) Coriolis Force (Fr) Friction Total Force acting on a body = mass times its acceleration (W)
ChemE 260 Conservation of Mass & Energy, Steady-State Processes April 15, 2005 Dr. William Baratuci Senior Lecturer Chemical Engineering Department University.
Modeling the Atmospheric Boundary Layer (2). Review of last lecture Reynolds averaging: Separation of mean and turbulent components u = U + u’, = 0 Intensity.
GEOGRAPHY 3015A. IT WAS AN INTERESTING SUMMER!
EVAT 554 OCEAN-ATMOSPHERE DYNAMICS FILTERING OF EQUATIONS FOR OCEAN LECTURE 10 (Reference: Peixoto & Oort, Chapter 3,8)
EVAT 554 OCEAN-ATMOSPHERE DYNAMICS FILTERING OF EQUATIONS OF MOTION FOR ATMOSPHERE (CONT) LECTURE 7 (Reference: Peixoto & Oort, Chapter 3,7)
EVAT 554 OCEAN-ATMOSPHERE DYNAMICS FILTERING OF EQUATIONS FOR ATMOSPHERE (CONT) LECTURE 6 (Reference: Peixoto & Oort, Chapter 3)
Richard Rotunno National Center for Atmospheric Research, USA Fluid Dynamics for Coastal Meteorology.
ERT 206/4 THERMODYNAMICS SEM 2 (2011/2012). light Energy can exist in numerous forms: Thermal Mechanical Kinetic Potential Electric Magnetic Chemical.
EVAT 554 OCEAN-ATMOSPHERE DYNAMICS
EVAT 554 OCEAN-ATMOSPHERE DYNAMICS SVERDRUP TRANSPORT LECTURE 15 (Reference: Peixoto & Oort, Chapter 8,10)
Investigation of Mixed Layer Depth in the Southern Ocean by using a 1-D mixed layer model Chin-Ying Chien & Kevin Speer Geophysical Fluid Dynamics Institute,
Richard Rotunno National Center for Atmospheric Research, USA Dynamical Mesoscale Mountain Meteorology.
EVAT 554 OCEAN-ATMOSPHERE DYNAMICS TIME-DEPENDENT DYNAMICS; WAVE DISTURBANCES LECTURE 21.
Evaporation Slides prepared by Daene C. McKinney Reading: Applied Hydrology Sections 4.1 and 4.2 Quotation for today (from Socrates) "There is only one.
FREE CONVECTION 7.1 Introduction Solar collectors Pipes Ducts Electronic packages Walls and windows 7.2 Features and Parameters of Free Convection (1)
EVAT 554 OCEAN-ATMOSPHERE DYNAMICS GYRE-SCALE OCEAN CIRCULATION LECTURE 16 (Reference: Peixoto & Oort, Chapter 8,10)
Chapter 5 - PBL MT 454 Material Based on Chapter 5 The Planetary Boundary Layer.
Quantification of the Infection & its Effect on Mean Fow.... P M V Subbarao Professor Mechanical Engineering Department I I T Delhi Modeling of Turbulent.
Conservation of Salt: Conservation of Heat: Equation of State: Conservation of Mass or Continuity: Equations that allow a quantitative look at the OCEAN.
Chapter 9: Natural Convection
INTRODUCTION TO CONVECTION
Basic dynamics ●The equations of motion and continuity Scaling Hydrostatic relation Boussinesq approximation ●Geostrophic balance in ocean’s interior.
Basic dynamics The equation of motion Scale Analysis
Energy and Matter. Energy Energy- the ability to do work such as moving matter a distance causing a heat transfer between two objects at different temperatures.
Lecture Guidelines for GEOF110 Chapter 7 Until Re-averaging + movie = 2 h scaling/ hydrostatic equation = 2 h Ilker Fer Guiding for blackboard presentation.
Evaporation What is evaporation? How is evaporation measured? How is evaporation estimated? Reading for today: Applied Hydrology Sections 3.5 and 3.6 Reading.
First law of thermodynamics Kishan Solanki(12me102) Patel manthan(12me132)
Meteorological Variables 1. Local right-hand Cartesian coordinate 2. Polar coordinate x y U V W O O East North Up Dynamic variable: Wind.
Surface LH, SH, and momentum drag are determined by turbulent transport near the surface.
Percent (%) Evaluation Attendance and Class Participation 5%
Atmospheric Thermodynamics: An Energy Perspective
EVAT 554 OCEAN-ATMOSPHERE DYNAMICS
General form of conservation equations
Reynolds-Averaged Navier-Stokes Equations -- RANS
EVAT 554 OCEAN-ATMOSPHERE DYNAMICS
ATOC 4720 class35 1. The thermodynamic energy equation
The Hadley Cell continued…
Conservation of Momentum (horizontal)
Presentation transcript:

EVAT 554 OCEAN-ATMOSPHERE DYNAMICS EQUATIONS OF MOTION (CONT); ENERGY EQUATION LECTURE 4 (Reference: Peixoto & Oort, Chapter 3)

Zonal Momentum Balance: Meridional Momentum Balance: Vertical Momentum Balance: Continuity

SIMPLIFYING APPROXIMATIONS 1. “Boussinesq Approximation” (accept in gravity or “buoyancy” term) 2. Ignore “Metric Terms” (terms that scale as 1/a are orders of magnitude smaller than other terms) 3. Assume equations averaged over e.g. several hours (replace molecular diffusion with Eddy Diffusion based on contribution of averaged non-linear terms)

Zonal Momentum Balance: Meridional Momentum Balance: Vertical Momentum Balance: Continuity: But this is not a closed set of equations!

First Law of Thermodynamics Energy is neither destroyed nor created, but changes form during ordinary physical and chemical processes CONSERVATION OF ENERGY Heating = Change in Internal Energy + Work Done

CONSERVATION OF ENERGY First Law of Thermodynamics Energy is neither destroyed nor created, but changes form during ordinary physical and chemical processes Heating = Change in Internal Energy + Work Done

Includes radiative heating, latent heating, frictional heating, conduction and turbulent heat flux (“diabatic” heating) Heating = Change in Internal Energy + Work Done CONSERVATION OF ENERGY First Law of Thermodynamics Energy is neither destroyed nor created, but changes form during ordinary physical and chemical processes

Heating = Change in Internal Energy + Work Done CONSERVATION OF ENERGY Example: How much energy is needed to warm 2 kg of dry air by 5 o C? m air = 2 kg,  T = 5 o C  Q H = m air C p  T= (2kg)(1005 J kg -1 K -1 )(5 o C) = kJ Cp = 1005 J kg-1 K-1 (dry air)

CONSERVATION OF ENERGY Define the heating rate,

CONSERVATION OF ENERGY Define the heating rate, Combine molecular and eddy diffusive heat transport:

CONSERVATION OF ENERGY Combine molecular and eddy diffusive heat transport:

CONSERVATION OF ENERGY

Boundary Terms

CONSERVATION OF ENERGY Planck Blackbody Incident Solar

We still do not have a closed system of equations! equation of state... Let us first consider the atmosphere…